 Its brightness varies with an amplitude of 0m.02 over a period of 0.3951 days.However, it is currently thought more likely to be a different type of variable, possibly a λ Eridani variable or rotating ellipsoidal variable.This object is a B-type main-sequence star with a stellar classification of B4 Vne, where the suffix notation indicates "nebulous" (broad) lines due to rapid rotation, along with emission lines from circumstellar material.